Defect-Driven Degradation of MXenes in Aqueous Environments and Mitigation Strategies: Insights from First-Principles.
basic_science · Level V
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- Record sourced from PubMed, PMID 41085334.
- Also identified by DOI 10.1021/acsnano.5c09946.
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Abstract
MXenes have attracted considerable attention due to their tunable surface chemistry, high electrical conductivity, and ease of solution processing, making them promising candidates for a wide array of applications. The inherent tendency of MXenes to degrade under environmental conditions constrains their compositional diversity and limits certain practical applications. Our computational study shows that degradation of defect-free Ti<sub>3</sub>C<sub>2</sub>T<sub><i>x</i></sub> is kinetically limited, whereas common defects markedly lower the activation barriers for water attack. Using ab initio molecular dynamics simulations (AIMD) combined with thermodynamic analysis, we show that titanium vacancies V<sub>Ti</sub> act as active sites for the protonation of subsurface carbon atoms, weakening the bonds with and accelerating the release of adjacent Ti atoms. Targeted passivation of these sites by adsorbed metal cations (e.g., Li<sup>+</sup>, Na<sup>+</sup>, K<sup>+</sup>, and Mg<sup>2+</sup>) is predicted to effectively mitigate degradation by suppressing protonation and increasing the barrier for Ti oxidation. This stabilization arises from two synergistic effects: (i) electronic structure modification driven by a strong dipole moment, which markedly shifts the work function, and (ii) steric hindrance that limits water access to reactive defect sites. We also demonstrate that carbon vacancies V<sub>C</sub> significantly destabilize adjacent Ti atoms, lowering the energy barrier for the water attack reaction. The substitution of V<sub>C</sub> with electronegative species such as O or N does not significantly improve the stability of Ti<sub>3</sub>C<sub>2</sub>T<sub><i>x</i></sub>, highlighting the detrimental role of any defects in the carbon sublattice. Because V<sub>C</sub> are typically inherited from the precursor phase and cannot be removed during postsynthesis, controlling their concentration during M<sub><i>n</i>+1</sub>AX<sub><i>n</i></sub> phases synthesis is essential. Our thermodynamic analysis reveals that A-rich (e.g., Al-rich) synthesis conditions substantially increase the formation energy of V<sub>C</sub> and V<sub>N</sub> defects in a large spectrum of M<sub><i>n</i>+1</sub>AX<sub><i>n</i></sub> phases, providing a generalizable strategy for defect suppression and improved durability of the resulting MXenes.